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Properties of dust in the martian atmosphere and its effect on temperature structure

✍ Scribed by J.B. Pollack

Publisher
Elsevier Science
Year
1982
Tongue
English
Weight
641 KB
Volume
2
Category
Article
ISSN
0273-1177

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## Mars Pathfinder made numerous discoveries, one of which was a deep temperature inversion that extended from about 15 km down to 8 km above the surface. It has been suggested by Haberle et al. (1999. J. Geophys. Res. 104, 8957-8974.) that radiative cooling by a water ice cloud may generate such